Origin of howardites, diogenites and eucrites: A mass balance constraint
- 28 February 1985
- journal article
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 49 (2) , 577-586
- https://doi.org/10.1016/0016-7037(85)90049-3
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Trace elements as quantitative probes of differentiation processes in planetary interiorsReviews of Geophysics, 1980
- REE patterns versus the origin of the basaltic achondritesIcarus, 1979
- Electromagnetic heating of minor planets in the early solar systemIcarus, 1979
- Mineral chemistry of layered Archaean anorthosite at Majorqap qâva, near Fiskenæsset, southwest GreenlandLithos, 1977
- Petrogenesis of eucrite, howardite and diogenite meteoritesNature, 1975
- NEW CHEMICAL ANALYSES OF SIX ACHONDRITES AND ONE CHONDRITEMeteoritics, 1974
- Origin of lunar feldspathic rocksEarth and Planetary Science Letters, 1973
- On the origin of eucrites and diogenitesEarth and Planetary Science Letters, 1973
- Densities of liquid silicate systems calculated from partial molar volumes of oxide componentsAmerican Journal of Science, 1970
- The system MgO-FeO-SiO 2American Journal of Science, 1935